Issue |
A&A
Volume 698, May 2025
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Article Number | C4 | |
Number of page(s) | 1 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/202555587e | |
Published online | 11 June 2025 |
Surface brightness discontinuities in radio halos
Insights from the MeerKAT Galaxy Cluster Legacy Survey (Corrigendum)
1
INAF – IRA, Via P. Gobetti 101, I-40129 Bologna, Italy
2
NASA/Goddard Space Flight Center, 8800 Greenbelt Rd, MD 20771, USA
3
Leiden Observatory, Leiden University, PO Box 9513 NL-2300 RA Leiden, The Netherlands
4
ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2 NL-7990 AA Dwingeloo, The Netherlands
⋆ Corresponding author: andrea.botteon@inaf.it
Key words: errata, addenda / acceleration of particles / radiation mechanisms: non-thermal / shock waves / galaxies: clusters: general / galaxies: clusters: intracluster medium
Due to a bug in the software used to extract the surface brightness profiles (PYPROFFIT), the profile shown in red in Fig. 3 of the original paper is incorrect. The correct profile is presented in Fig. 1 here, which shows that the surface brightness drops by a factor of ∼10 at the position of the discontinuity (instead of the factor of ∼6–7 originally reported). This was the only profile presented in the original paper affected by the bug in PYPROFFIT.
![]() |
Fig. 1. Corrected version of the profile reported in red in Fig. 3 of the original paper. |
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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All Figures
![]() |
Fig. 1. Corrected version of the profile reported in red in Fig. 3 of the original paper. |
In the text |
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